Observation of TeV gammm rays from NE-rim of SN1006 with CANGAROO-II 10m telescope

Details Observation of TeV gammm rays from NE-rim of SN1006 with CANGAROO-II 10m telescope Observation of TeV gammm rays from NE-rim of SN1006 with CANGAROO-II 10m telescope

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....6.2455h&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

2

Scientific paper

Observation of the North East (NE) rim of SN1006 has been carried out using the CANGAROO-II 10m telescope in April and May 2000. The observation time is 55.2 and 48.8 hours, ONand OFF-source runs, respectively. We have confirmed TeV Gamma-ray emission from the NE-rim. The energy threshold of the observed flux is estimated to be around 1 TeV by the Monte Carlo simulation assuming the inverse Compton like spectrum. The preliminary flux is consistent with the previous result observed by the 3.8m CANGAROO telescope.

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